Program
Monday, December 11, 2023
| Time |
Event |
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09:00 - 10:00
|
Coffee break (Hall) |
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10:00 - 12:10
|
Galaxy formation from 1 to 14 Gyr (Amphitheatre) - Joop Schaye |
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10:00 - 10:10 |
› Welcome - Yohan Dubois, IAP |
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10:10 - 10:50 |
› Simulating populations of galaxies and their details from the end of the Reionization to the current epoch - Annalisa Pillepich, Max Planck Society (GERMANY) |
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10:50 - 11:10 |
› Calibrating subgrid feedback in cosmological simulations that include a cold interstellar gas phase - Evgenii Chaikin, Leiden Observatory, Leiden University |
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11:10 - 11:30 |
› On the universality of star formation efficiency across time - Alvaro Segovia Otero, Lund Observatory |
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11:30 - 11:50 |
› The interplay of magnetism, radiation and cosmic rays in dwarf galaxy formation - Sergio Martin-Alvarez, Kavli Institute for Particle Astrophysics and Cosmology |
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11:50 - 12:10 |
› Introducing the NewCluster simulation - Sukyoung Yi, Yonsei University |
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12:10 - 13:40
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Lunch |
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13:40 - 15:40
|
Galaxy formation from 1 to 14 Gyr (Amphitheatre) - Annalisa Pillepich |
(+)
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13:40 - 14:00 |
› Revisiting the Missing Satellite Problem and Starless Subhalos - Seyoung Jeon, Yonsei University |
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14:00 - 14:20 |
› On the origin of star formation quenching of galaxies in group environments using NewHorizon - Jinsu Rhee, Korea Astronomy and Space science Institute |
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14:20 - 14:40 |
› Why does the absence of mergers mater? - Florent Renaud, Strasbourg Observatory |
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14:40 - 15:00 |
› The surprisingly rapid emergence of strong bars in primordial star-forming galaxies - Frédéric Bournaud, AIM/CEA Paris-Saclay |
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15:00 - 15:20 |
› Star formation across main sequence and quenched galactic environments - Sarah Jeffreson, Harvard-Smithsonian Center for Astrophysics |
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15:20 - 15:40 |
› Molecular gas in low metallicity galaxies and its implications for star formation - Ava Polzin, University of Chicago |
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15:40 - 16:25
|
Coffee break (Hall & Entresol) |
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16:25 - 18:05
|
Galaxy formation from 1 to 14 Gyr (Amphitheatre) - Annalisa Pillepich |
(+)
|
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16:25 - 16:45 |
› Universality of gravitation-driven isothermal turbulence in galactic disks - Jeremy Fensch, CRAL |
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16:45 - 17:05 |
› Emergence and cosmic evolution of the Kennicutt-Schmidt relation driven by interstellar turbulence - Katarina Kraljic, Observatoire astronomique de Strasbourg |
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17:05 - 17:25 |
› The GigaEris Simulation: probing the evolution of disc galaxies evolution at Redshift > 4 - Floor Van Donkelaar, Institute for Computational Science, University of Zurich |
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17:25 - 17:45 |
› Morphology of High-Redshift Galaxies in the Horizon Run 5 Simulation and JWST Observation - Changbom Park, Korea Institute for Advanced Study |
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17:45 - 18:05 |
› Three Eras of Computational Cosmology - August Evrard, University of Michigan |
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18:05 - 21:00
|
Cocktail (Hall & Entresol) |
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Tuesday, December 12, 2023
| Time |
Event |
(+)
|
|
09:00 - 10:40
|
Galaxies in the first Gyr (Amphitheatre) - Stefanie Walch |
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|
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09:00 - 09:40 |
› Galaxies in the first Gyr: Frontiers of both theory and observation - Harley Katz, University of Oxford |
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|
09:40 - 10:00 |
› Early Galaxy Formation and Cosmic Reionization in the JWST Era - Hakim Atek, Institut d'Astrophysique de Paris |
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10:00 - 10:20 |
› Pitfalls of numerical simulations in the JWST era. - Andrea Pallottini, Scuola Normale Superiore |
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10:20 - 10:40 |
› New Simulations of Feedback-Free Starbursts at Cosmic Dawn - Avishai Dekel, The Hebrew University of Jerusalem |
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10:40 - 11:10
|
Coffee break (Hall & Entresol) |
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11:10 - 12:30
|
Galaxies in the first Gyr (Amphitheatre) - Stefanie Walch |
(+)
|
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11:10 - 11:30 |
› Bursty star formation in galaxies at cosmic dawn from cosmological zoom-in simulations - Guochao Sun, Northwestern University |
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11:30 - 11:50 |
› Simulating Cosmic Reionization on all scales - Ilian Iliev, Astronomy Centre, University of Sussex |
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11:50 - 12:10 |
› Dusty galaxies powering Reionization in Cosmic Dawn III - Joseph Lewis, Universität Heidelberg, Max Planck Institute for Astronomy |
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12:10 - 12:30 |
› SPICE : Connecting the effect of stellar feedback in first galaxies and cosmic reionisation - Aniket Bhagwat, Max-Planck-Institut für Astrophysik |
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12:30 - 14:00
|
Lunch |
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14:00 - 15:40
|
Are cosmic rays a missing ingredient? (Amphitheatre) - Thorsten Naab |
(+)
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14:00 - 14:40 |
› Cosmic Ray Feedback from Supernovae to Galaxy Clusters - Mateusz Ruszkowski, Department of Astronomy, University of Michigan-Ann Arbor |
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14:40 - 15:00 |
› Cosmic-ray diffusion and the multi-phase interstellar medium in a dwarf galaxy. I. Large-scale properties and γ-ray luminosities - Arturo Nuñez-Castiñeyra, CEA- Saclay |
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15:00 - 15:20 |
› A multi-frequency view on simulating galaxy formation with cosmic rays - Maria Werhahn, Max Planck Institute for Astrophysics |
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15:20 - 15:40 |
› Cosmic ray feedback and magnetic dynamos in galaxies - Christoph Pfrommer, Leibniz Institute for Astrophysics Potsdam |
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15:40 - 16:25
|
Coffee break (Hall & Entresol) |
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16:25 - 17:05
|
Are cosmic rays a missing ingredient? (Amphitheatre) - Thorsten Naab |
(+)
|
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16:25 - 16:45 |
› Comic ray-supported Galactic Outflows: Probing kinematics and multiphase gas strucutre within ISM simulations - Tim-Eric Rathjen, University of Cologne |
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16:45 - 17:05 |
› The impact of cosmic rays on the outflow production and composition - Nicolas Peschken, Galileo Galilei Institute for Theoretical Physics |
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17:05 - 18:05
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Can we make robust predictions about dust? (Amphitheatre) - Thorsten Naab |
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17:05 - 17:25 |
› Dusty, star-forming galaxies at z=2: Can simulations reproduce these extreme galaxies? - Andrea Gebek, Universiteit Gent = Ghent University |
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17:25 - 17:45 |
› Modelling early massive dusty galaxies and their properties with the Obelisk simulation - Maxime Trebitsch, Kapteyn Astronomical Institute |
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Wednesday, December 13, 2023
| Time |
Event |
(+)
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09:00 - 10:40
|
Galaxies in non-standard cosmologies (Amphitheatre) - Volker Springel |
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09:00 - 09:40 |
› Galaxy formation in non-standard cosmological models - Baojiu Li, Durham University |
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09:40 - 10:00 |
› The impact of Baryons vs. Self-Interacting Dark Matter on Galaxy Formation - Camila Correa, CEA Paris-Saclay |
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10:00 - 10:20 |
› Galaxy formation and primordial non-Gaussianities - Clément Stahl, Observatoire astronomique de Strasbourg |
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10:20 - 10:40
|
Large-scale structures and galaxies (Amphitheatre) - Volker Springel |
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10:20 - 10:40 |
› Towards constraining the gas properties in the cosmic web - Yan-Chuan Cai, Institute for Astronomy, University of Edinburgh |
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10:40 - 11:10
|
Coffee break (Hall & Entresol) |
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11:10 - 12:30
|
Large-scale structures and galaxies (Amphitheatre) - Volker Springel |
(+)
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11:10 - 11:30 |
› Constraints on particle dark matter using the Intergalactic Medium - Matteo VIEL, Scuola Internazionale Superiore di Studi Avanzati / International School for Advanced Studies |
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11:30 - 11:50 |
› the cosmic web - CGM interface from Milky Ways to Clusters - Charlotte Welker, City University of New York |
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11:50 - 12:10 |
› Flows around galaxies: I. The dependence of galaxy connectivity on cosmic environments and effects on the star formation rate - Daniela Galárraga-Espinosa, Max Planck Institute for Astrophysics |
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12:10 - 12:30 |
› On the causal origin of dark matter halo and galaxy angular momentum: replacing galaxies in their cosmological context - Corentin Cadiou, Division of Astrophysics, Department of Physics [Lund University], IAP |
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12:30 - 14:00
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Lunch |
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14:00 - 18:00
|
Nick Kaiser Tribute (Amphitheatre) |
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18:00 - 20:00
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Cocktail (Hall & Forum) |
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20:00 - 23:00
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Conference Dinner (Madame Brasserie - Tour Eiffel) |
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Thursday, December 14, 2023
| Time |
Event |
(+)
|
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09:40 - 11:00
|
Large-scale structures and galaxies (Amphitheatre) - Harley Katz |
(+)
|
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09:40 - 10:20 |
› Simulations at the interface between large-scale structure and galaxy formation - Joop Schaye, Leiden Observatory, Leiden University |
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10:20 - 10:40 |
› The FLAMINGO suite of cosmological simulations - Schaller Matthieu, Lorentz Institute |
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10:40 - 11:00 |
› Galaxy groups and clusters in FLAMINGO - Joey Braspenning, Leiden Observatory |
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11:00 - 11:30
|
Coffee break (Hall & Entresol) |
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11:30 - 12:30
|
The nature of the circum-galactic medium (Amphitheatre) - Harley Katz |
(+)
|
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11:30 - 12:10 |
› The multi-scale multi-phase Circum-Galactic Medium - Celine Peroux, European Southern Observatory |
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12:10 - 12:30 |
› Resolving the physics of multi-scale gaseous halos - Dylan Nelson, Heidelberg University |
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12:30 - 14:00
|
Lunch |
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14:00 - 15:40
|
The nature of the circum-galactic medium (Amphitheatre) - Sukyoung Yi |
(+)
|
|
14:00 - 14:20 |
› Constraining feedback processes with the circum-galactic medium - Maxime Rey, Yonsei University |
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14:20 - 15:00 |
› Arkenstone: A Multi-Scale Approach to Galaxy Formation - Drummond Fielding, Center for Computational Astrophysics, Flatiron Institute |
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15:00 - 15:20 |
› Unraveling Multiphase Dynamics: Stirring the Magnetic spaghetti in a Turbulent sauce - Hitesh Kishore Das, Max Planck Institute for Astrophysics |
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15:20 - 15:40 |
› The origin of multiphase galactic outflows - Ulrich Steinwandel, Center for Computational Astrophysics (CCA, Simons Foundation) |
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|
15:40 - 16:25
|
Coffee break (Hall & Entresol) |
|
|
16:25 - 17:05
|
The nature of the circum-galactic medium (Amphitheatre) - Sukyoung Yi |
(+)
|
|
16:25 - 16:45 |
› Confronting Lyman alpha profiles of high-z galaxies with simulations with strong stellar feedback - Taysun Kimm, Yonsei University |
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16:45 - 17:05 |
› Constraining the flows of gas around galaxies with Lyman-alpha observations -- insights from simulations - Jeremy Blaizot, Centre de Recherche Astrophysique de Lyon |
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17:05 - 18:05
|
Feedback from active galactic nuclei (Amphitheatre) - Sukyoung Yi |
(+)
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17:05 - 17:25 |
› The kinematics and observable properties of AGN jets and cavities with cosmological simulations - Laura Di Federico, Universitäts-Sternwarte München, Ludwig-Maximilians-Universität |
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17:25 - 17:45 |
› The Significance of Recycled Gas: The Primary Fuel for SMBH Accretion in Cosmological Simulations - Ena Choi, University of Seoul |
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|
17:45 - 18:05 |
› Multimessenger study of merging massive black holes in the Obelisk simulation: gravitational waves, electromagnetic counterparts, and their link to galaxy and black hole populations - Chi An Dong Páez, Institut d'Astrophysique de Paris |
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Friday, December 15, 2023
| Time |
Event |
(+)
|
|
09:00 - 10:40
|
Feedback from active galactic nuclei (Amphitheatre) - Marta Volonteri |
(+)
|
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09:00 - 09:40 |
› Feedback from AGN: Physics & Numerics - Tiago Costa, Newcastle University |
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09:40 - 10:00 |
› GRMHD Simulations Meet Galactic Evolution: A Refined Model for AGN Feedback - Ivan Almeida, Newcastle University [Newcastle], Instituto de Astronomia, Geofísica e Ciências Atmosféricas [São Paulo] |
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|
10:00 - 10:20 |
› New hyper-refinement simulations for long-standing problems in black hole-galaxy coevolution - Daniel Angles-Alcazar, University of Connecticut |
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10:20 - 10:40 |
› Super-Eddington accretion during early black hole growth - Brian Jiang, University of Cambridge [UK] |
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10:40 - 11:10
|
Coffee break (Hall & Entresol) |
|
|
11:10 - 12:30
|
Feedback from active galactic nuclei (Amphitheatre) - Marta Volonteri |
(+)
|
|
11:10 - 11:30 |
› Settling SMBH at the center of galaxies in the simulation - San Han, Yonsei University |
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|
11:30 - 11:50 |
› High-performance galaxy formation simulations with accurate massive black hole dynamics - Antti Rantala, Max Planck Institute for Astrophysics |
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11:50 - 12:10 |
› Intermediate mass black hole feedback in dwarf galaxy simulations with a resolved ISM and accurate nuclear stellar dynamics - Christian Partmann, Max-Planck-Institut für Astrophysik |
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12:10 - 12:30 |
› AGN in Clumpy DisCs (ACDC): How does ISM structure shape multiphase outflows? - Samuel Ward, European Southern Observatory, Newcastle University |
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12:30 - 14:00
|
Lunch (Amphitheatre) |
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14:00 - 15:20
|
Feedback from stars (Amphitheatre) - Romain Teyssier |
(+)
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14:00 - 14:40 |
› Feedback from stars - Thorsten Naab, Max Planck Institute for Astrophysics |
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|
14:40 - 15:00 |
› Multi-phase gas in cosmological galaxy formation simulations - Rainer Weinberger, Leibniz Institute for Astrophysics Potsdam |
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15:00 - 15:20 |
› Simulating the formation of globular clusters and their multiple populations in low-metallicity dwarf galaxies - Natalia Lahén, Max Planck Institute for Astrophysics |
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15:20 - 15:50
|
Coffee break (Hall & Entresol) |
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|
15:50 - 17:10
|
Feedback from stars (Amphitheatre) - Romain Teyssier |
(+)
|
|
15:50 - 16:30 |
› The exciting (and uncertain) world of modeling dust in galaxy simulations - Desika Narayanan, University of Florida |
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16:30 - 16:50 |
› Radiation-hydrodynamic simulations of dwarf galaxies with metallicity dependent feedback from individual stars - Yunwei Deng, Department of Astronomy, Tsinghua University |
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16:50 - 17:10 |
› Resolved AGN disks in cosmological zoom simulations - Norman Murray, Canadian Institute for Theoretical Astrophysics (CITA), University of Toronto |
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